Search Results
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data set:
KECK II ESI IMAGES OF 81P/WILD 2
CCD images of comet 81P/Wild 2 taken 2003 December 19-21 UT with the ESI instrument on Keck II in support of the Stardust encounter.
SUPPORT ARCHIVES - EAR-C-I0039-2-SBN0007/KECKIIESI-V1.0 - starting 2003-12-19T00:00:00Z -
data set:
SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC V1.0
A 2004-2008 spectroscopic survey of asteroids selected as V-type candidates based on their Sloan Digital Sky Survey Moving Object Catalog colors.
SUPPORT ARCHIVES - EAR-A-I0039/I0576-4-SDSSMOCVSPEC-V1.0 - starting 2004-11-10T08:13:00Z -
data set:
IANNINI ASTEROID FAMILY SPECTRA V1.0
Spectra obtained from 2004 through 2007 of members of the Iannini asteroid family.
SUPPORT ARCHIVES - EAR-A-I0039-4-IANNINISPEC-V1.0 - starting 2004-11-10T05:35:00Z -
instrument:
KECK ECHELLE SPECTROGRAPH AND IMAGER for OBS378T2
Information about the KECK ECHELLE SPECTROGRAPH AND IMAGER for OBS378T2 instrument -
collection:
document collection for the "SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC" bundle
This is the document collection for the gbo.ast-v-type.moscovitz.spectra bundle. These data are the results of a spectroscopic survey designed to target and detect asteroids whose photometric colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. The colors of these candidates were measured as part of the 3rd release of the Sloan Digital Sky Survey Moving Object Catalog (Ivezic et al. 2001) [IVEZICETAL2001]. These spectra were obtained with two visible wavelength instruments: the Echellete Spectrograph and Imager (ESI, Sheinis et al. 2002) [SHEINISETAL2002] on Keck II and the Supernova Integral Field Spectrograph (SNIFS, Lantz et al. 2004) [LANTZETAL2004] at the University of Hawaii 2.2m telescope. A subset of these data were published in Moskovitz et al. (2008a, 2008b) [MOSKOVITZETAL2008, MOSKOVITZETAL2008B]. -
collection:
browse collection for the "IANNINI ASTEROID FAMILY SPECTRA" bundle
This is the browse collection for the gbo.ast-iannini-family.spectra bundle. Keck/ESI spectra of 11 Iannini asteroid family members were obtained over visual wavelengths. The data have been published in Willman, et al. (2008Icar...195...663W)[WILLMANETAL2008]. The spectra show family likeness and are believed to represent young S class surfaces aged a few million years by space weathering, the dynamically estimated collisional age of the family. -
bundle:
SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC
These data are the results of a spectroscopic survey designed to target and detect asteroids whose photometric colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. The colors of these candidates were measured as part of the 3rd release of the Sloan Digital Sky Survey Moving Object Catalog (Ivezic et al. 2001) [IVEZICETAL2001]. These spectra were obtained with two visible wavelength instruments: the Echellete Spectrograph and Imager (ESI, Sheinis et al. 2002) [SHEINISETAL2002] on Keck II and the Supernova Integral Field Spectrograph (SNIFS, Lantz et al. 2004) [LANTZETAL2004] at the University of Hawaii 2.2m telescope. A subset of these data were published in Moskovitz et al. (2008a, 2008b) [MOSKOVITZETAL2008, MOSKOVITZETAL2008B]. -
instrument:
Keck Echelle Spectrograph and Imager
Information about the Keck Echelle Spectrograph and Imager instrument -
bundle:
IANNINI ASTEROID FAMILY SPECTRA
Keck/ESI spectra of 11 Iannini asteroid family members were obtained over visual wavelengths. The data have been published in Willman, et al. (2008Icar...195...663W)[WILLMANETAL2008]. The spectra show family likeness and are believed to represent young S class surfaces aged a few million years by space weathering, the dynamically estimated collisional age of the family. -
collection:
data collection for the "IANNINI ASTEROID FAMILY SPECTRA" bundle
This is the data collection for the gbo.ast-iannini-family.spectra bundle. Keck/ESI spectra of 11 Iannini asteroid family members were obtained over visual wavelengths. The data have been published in Willman, et al. (2008Icar...195...663W)[WILLMANETAL2008]. The spectra show family likeness and are believed to represent young S class surfaces aged a few million years by space weathering, the dynamically estimated collisional age of the family. -
collection:
browse collection for the "SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC" bundle
This is the browse collection for the gbo.ast-v-type.moscovitz.spectra bundle. These data are the results of a spectroscopic survey designed to target and detect asteroids whose photometric colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. The colors of these candidates were measured as part of the 3rd release of the Sloan Digital Sky Survey Moving Object Catalog (Ivezic et al. 2001) [IVEZICETAL2001]. These spectra were obtained with two visible wavelength instruments: the Echellete Spectrograph and Imager (ESI, Sheinis et al. 2002) [SHEINISETAL2002] on Keck II and the Supernova Integral Field Spectrograph (SNIFS, Lantz et al. 2004) [LANTZETAL2004] at the University of Hawaii 2.2m telescope. A subset of these data were published in Moskovitz et al. (2008a, 2008b) [MOSKOVITZETAL2008, MOSKOVITZETAL2008B]. -
collection:
document collection for the "IANNINI ASTEROID FAMILY SPECTRA" bundle
This is the document collection for the gbo.ast-iannini-family.spectra bundle. Keck/ESI spectra of 11 Iannini asteroid family members were obtained over visual wavelengths. The data have been published in Willman, et al. (2008Icar...195...663W)[WILLMANETAL2008]. The spectra show family likeness and are believed to represent young S class surfaces aged a few million years by space weathering, the dynamically estimated collisional age of the family. -
collection:
data collection for the "SPECTRA OF V-TYPE CANDIDATES FROM THE SDSS MOC" bundle
This is the data collection for the gbo.ast-v-type.moscovitz.spectra bundle. These data are the results of a spectroscopic survey designed to target and detect asteroids whose photometric colors are similar to those of Vesta family members and thus may be considered as candidates for having a basaltic composition. The colors of these candidates were measured as part of the 3rd release of the Sloan Digital Sky Survey Moving Object Catalog (Ivezic et al. 2001) [IVEZICETAL2001]. These spectra were obtained with two visible wavelength instruments: the Echellete Spectrograph and Imager (ESI, Sheinis et al. 2002) [SHEINISETAL2002] on Keck II and the Supernova Integral Field Spectrograph (SNIFS, Lantz et al. 2004) [LANTZETAL2004] at the University of Hawaii 2.2m telescope. A subset of these data were published in Moskovitz et al. (2008a, 2008b) [MOSKOVITZETAL2008, MOSKOVITZETAL2008B].
Data Sets and Information